Results 61 to 70 of about 96 (81)
Stellar Variability toward the Galactic Open Cluster NGC 7209
We present the analysis of stellar variability in an open cluster NGC 7209 using optical V -band CCD photometric observations. Out of 4499 stars in our study, we detected 284 candidate variables, including one identified previously.
Dorothy M. Mwanzia+10 more
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Resolving Pleiades Binary Stars with Gaia and Speckle Interferometric Observations
The Pleiades is the most prominent open star cluster visible from Earth and an important benchmark for simple stellar populations unified by common origin, age, and distance.
Dmitry Chulkov+2 more
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A Close Binary Lens Revealed by the Microlensing Event Gaia20bof
During the last 25 yr, hundreds of binary stars and planets have been discovered toward the Galactic bulge by microlensing surveys. Thanks to a new generation of large-sky surveys, it is now possible to regularly detect microlensing events across the ...
E. Bachelet+27 more
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ICCD Speckle Observations of Binary Stars. XIX. An Astrometric/Spectroscopic Survey of O Stars [PDF]
Brian D. Mason+5 more
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The large number of exoplanets discovered with the Transiting Exoplanet Survey Satellite (TESS) means that any observational biases from TESS could influence the derived stellar multiplicity statistics of exoplanet host stars. To investigate this problem,
Colin Littlefield+8 more
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Given that secular perturbations in a binary system not only excite high orbital eccentricities but also alter the planetary orbital inclination, the classical Keplerian orbital model is no longer applicable for orbital retrieval.
Xiumin Huang+6 more
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The long-duration Galactic-bulge microlensing event OGLE-2011-BLG-0462 produced relativistic astrometric deflections of the source star, which we measured using Hubble Space Telescope (HST) observations taken at eight epochs over ∼6 yr.
Kailash C. Sahu+9 more
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Ba Enrichment in Gaia MS+WD Binaries: Tracing s-process Element Production
A large population of intermediate-separation binaries, consisting of a main-sequence (MS) star and a white dwarf (WD), recently emerged from Gaia’s third data release (DR3), posing challenges to current models of binary evolution. Here we examine the s -
Param Rekhi+5 more
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Astrometric and photometric measurements of binary stars with adaptive optics: observations from 2001 to 2006 [PDF]
Lewis C. Roberts, Brian D. Mason
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Hidden Companions to Intermediate-mass Stars. XIX. Spin–Orbit Misalignment and a 0.26M ⊙, 1.8 au Companion in the Astrometric Binary Gamma Trianguli Australis* [PDF]
Idel Waisberg, Ygal Klein, Boaz Katz
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